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Volumn 562, Issue 1 PART I, 2001, Pages 297-302

Using pulsars to detect massive black hole binaries via gravitational radiation: Sagittarius A* and nearby galaxies

Author keywords

Black hole physics; Galaxy: center Gravitational waves; Radio continuum: general

Indexed keywords


EID: 0041349096     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/323491     Document Type: Article
Times cited : (72)

References (16)
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    • Detweiler, S.1
  • 10
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    • Doeleman, S.S.1
  • 12
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    • Unsolved Problems of the Milky Way, ed. L. Blitz, P. Teuben (Dordrecht: Kluwer)
    • Falcke, H. 1996, In IAU Symp. 169, Unsolved Problems of the Milky Way, ed. L. Blitz, P. Teuben (Dordrecht: Kluwer), 169
    • (1996) IAU Symp. , vol.169 , pp. 169
    • Falcke, H.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.